会议专题

UNCERTAINTIES OF TH/EU AND TH/HF CHRONOMETERS FROM NUCLEAR MASSES

The age of the Universe is one of the most important physical quantities in cosmology and it can be determined with the r-process nucleochronometer. Based on the classical r-process model, the r-process abundance patterns and various nuclear chronometers in the metal-poor halo stars are investigated by employing the newly developed nuclear mass models. It is found that the uncertainty of Th/Eu chronometer caused by nuclear mass uncertainties is about 4 Gyr, while the uncertainty of Th/Hf chronometer is so large that it should be taken with caution. With the Th/Eu chronometer, the age of the metal-poor stars CS 31082-001 is determined as 16.3 ±7.1 Gyr, which agrees well with the results derived from Th/U chronometer.

Nuclear chronometer r-process metal-poor star

Z. M. NIU B. SUN J. MENG

State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijin School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China Justus-L State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijin

国际会议

The 13th National Conference on Nuclear Structure(第十三届全国核结构研讨会暨第九次全国“核结构与量子力学专题讨论会

赤峰

英文

159-164

2010-07-24(万方平台首次上网日期,不代表论文的发表时间)